12 December 2024
University of Oslo, Oslo, Norway
Europe/Oslo timezone

Light nuclei production in Au+Au collisions at BES-II energies using the STAR detector

Not scheduled
20m
Kristan Birkeland auditorium, Department of Physics, University of Oslo, Oslo, Norway. (University of Oslo, Oslo, Norway)

Kristan Birkeland auditorium, Department of Physics, University of Oslo, Oslo, Norway.

University of Oslo, Oslo, Norway

Speaker

Sibaram Behera (IISER Tirupati)

Description

In heavy-ion collisions, the production mechanism of light (anti-)nuclei can be explained by either the thermal model or the coalescence model. By studying the yields and yield ratios of the light (anti-)nuclei, we can gain a better understanding of their production mechanisms and the properties of the expanding system during freeze-out. Additionally, it has been proposed that the enhancement of light nuclei compound ratios, e.g. $N_{t}N_{p}/N_{d}^{2}$ and $N_{^4He}N_{p}/N_{^3He}N_{d}$, with respect to the coalescence baseline could serve as a probe of critical phenomena in the QCD phase diagram.

In the first phase of the Beam Energy Scan (BES-I) program at RHIC, an enhancement relative to the coalescence baseline of the light nuclei yield ratio ($N_{t}N_{p}/N_{d}^{2}$) was observed in the most central Au+Au collisions at $\sqrt{s_{NN}}$ = 19.6 and 27 GeV, with a combined significance of 4.1$\sigma$. The precision of the new measurements will be significantly improved by the large data sets ($\sim10\times$ BES-I) obtained by the STAR BES-II with upgraded detector capabilities.

In this talk, we will present the centrality and energy dependence of transverse momentum ($p_T$) spectra of $p$, $\bar{p}$, $d$, $\bar{d}$, and $^{3}He$ in Au+Au collisions at BES-II energies of $\sqrt{s_{NN}}$ = 7.7 - 27 GeV. We will also report on the centrality and energy dependence of integrated particle yields ($dN/dy$) and mean $p_T$ ($\langle p_T \rangle$) of light nuclei. Furthermore, we will discuss the centrality and $p_T$ dependence of the coalescence parameters ($B_{2}(d)$ and $B_{3}(^3He)$). The physics implications of these results will be discussed.

Details

Name - Sibaram Behera
Title - Doctoral student
Institution name - Indian Institute of Science Education and Research (IISER), Tirupati
Country - India
Webpage of institution - https://www.iisertirupati.ac.in/

Internet talk Yes
Is this an abstract from experimental collaboration? Yes
Name of experiment and experimental site STAR Experiment, Brookhaven National Laboratory, USA
Is the speaker for that presentation defined? Yes

Author

Sibaram Behera (IISER Tirupati)

Presentation materials

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